Hostname: page-component-586b7cd67f-t7czq Total loading time: 0 Render date: 2024-11-28T16:46:29.223Z Has data issue: false hasContentIssue false

Early results from the SAGE-SMC Spitzer legacy

Published online by Cambridge University Press:  01 July 2008

Karl D. Gordon
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
M. Meixner
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
R. D. Blum
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
W. Reach
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
B. A. Whitney
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
J. Harris
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
R. Indebetouw
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. D. Bolatto
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
J.-P. Bernard
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
M. Sewilo
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
B. L. Babler
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
M. Block
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
C. Bot
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. Bracker
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
L. Carlson
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
E. Churchwell
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
G. C. Clayton
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
M. Cohen
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
C. W. Engelbracht
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
Y. Fukui
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
V. Gorjian
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. Hony
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
J. L. Hora
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
F. Israel
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. Kawamura
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. K. Leroy
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. Li
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. Madden
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. R. Marble
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
F. Markwick-Kemper
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
M. Meade
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
K. A. Misselt
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. Mizuno
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
N. Mizuno
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
E. Muller
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
J. M. Oliveira
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
K. Olsen
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
T. Onishi
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
R. Paladini
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
D. Paradis
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. Points
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
T. Robitaille
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
D. Rubin
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
K. M. Sandstrom
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. Sato
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
H. Shibai
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
J. D. Simon
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
L. J. Smith
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. Srinivasan
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
A. G. G. M. Tielens
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
U. P. Vijh
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
S. van Dyk
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
J. Th. van Loon
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
K. Volk
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
D. Zaritsky
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA email: kgordon@stsci.edu
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Early results from the SAGE-SMC (Surveying the Agents of Galaxy Evolution in the tidally-disrupted, low-metallicity Small Magellanic Cloud) Spitzer legacy program are presented. These early results concentrate on the SAGE-SMC MIPS observations of the SMC Tail region. This region is the high H i column density portion of the Magellanic Bridge adjacent to the SMC Wing. We detect infrared dust emission and measure the gas-to-dust ratio in the SMC Tail and find it similar to that of the SMC Body. In addition, we find two embedded cluster regions that are resolved into multiple sources at all MIPS wavelengths.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2009

References

Bolatto, A. D., Simon, J. D., Stanimirović, S., et al. 2007, ApJ, 655, 212CrossRefGoogle Scholar
Bot, C., Boulanger, F., Lagache, G., Cambrésy, L., & Egret, D. 2004, A&A, 423, 567Google Scholar
Connors, T. W., Kawata, D., & Gibson, B. K. 2006, MNRAS, 371, 108CrossRefGoogle Scholar
Harris, J. 2007, ApJ, 658, 345CrossRefGoogle Scholar
Lee, J.-K., Rolleston, W. R. J., Dufton, P. L., & Ryans, R. S. I. 2005, A&A, 429, 1025Google Scholar
Meixner, M., Gordon, K. D., Indebetouw, R., et al. 2006, AJ, 132, 2268CrossRefGoogle Scholar